1977
DOI: 10.1103/physrevc.16.2296
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Photofission ofTh232with 9, 15, and 38 MeV peak bremsstrahlung

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Cited by 19 publications
(13 citation statements)
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“…The calculation of saddle point configurations against the mass asymmetric deformation by Moller [95] showed a different type of potential barrier for 232 Th compared to 238 U, which was mentioned before. Thus, the observation of a triple humped mass distribution from the present and earlier work in bremsstrahlung [59,60], re- Table 3 Nuclear spectroscopic data and yields of fission products in the 10 MeV bremsstrahlung-induced fission of 240 Pu. actor neutron- [14][15][16] and mono-energetic neutron-induced [38][39][40][41][42] fission of 232 Th compared to that of 238 U and 240 Pu is due to a different type of potential barrier.…”
Section: Discussionmentioning
confidence: 63%
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“…The calculation of saddle point configurations against the mass asymmetric deformation by Moller [95] showed a different type of potential barrier for 232 Th compared to 238 U, which was mentioned before. Thus, the observation of a triple humped mass distribution from the present and earlier work in bremsstrahlung [59,60], re- Table 3 Nuclear spectroscopic data and yields of fission products in the 10 MeV bremsstrahlung-induced fission of 240 Pu. actor neutron- [14][15][16] and mono-energetic neutron-induced [38][39][40][41][42] fission of 232 Th compared to that of 238 U and 240 Pu is due to a different type of potential barrier.…”
Section: Discussionmentioning
confidence: 63%
“…In the electromagnetic fission of lighter actinides [52][53][54], higher yields of fission products around mass numbers 133-135 corresponding to a most probable charge of 52 have been observed. Similarly, higher yields of fission products around mass numbers 133-135 in the 3 and 14 MeV mono-energetic neutron-induced [28][29][30][31][32][33][34] and in the 9, 15 and 31 MeV bremsstrahlunginduced [59] fission of 232 Th have also been observed earlier. However, in the 6.44-13.13 MeV bremsstrahlung-induced fission of 232 Th [60], yields of fission products are more pronounced around mass numbers 143-145 compared to mass numbers 133-135, which is contradictory to the earlier observations [23][24][25][26][27]59].…”
Section: Introductionmentioning
confidence: 50%
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“…Only using future high duty cycle electron accelerators these difficulties can be avoided by constructing intense mono-energetic "tagged photon" sources or by doing (e, e'f)-coincidence experiments. In the past some photofission measurements of mass distributions had been performed with radiochemical methods and catcher foil techniques on 232Th and 238U for different bremsstrahlung endpoint energies (see [4,5] …”
Section: * Partially Supported By the Deutsche Forschungsgemeinschaftmentioning
confidence: 99%